The onset of star formation in primordial haloes | Astronomy & Astrophysics (A&A)

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Table 1:

Parameters adopted for the simulations.
Model	Number of	$M_{\rm gas}\rm$	$M_{\rm dm}\rm$	$\Omega_{0{\rm M}}$	$\Omega_{0\Lambda}$	$\Omega_{0{\rm b}}$	h	$\sigma_8$	n	SF threshold
	gas+dm particles	$[ M_{\odot}/{\it h}]$	$[ M_{\odot}/{\it h}]$							$[h^2~\rm cm^{-3}]$
wmap5-ht	$2\times 32~768~000$	128	621	0.258	0.742	0.0441	0.72	0.8	0.96	135.0
wmap5-lt	$2\times 32~768~000$	128	621	0.258	0.742	0.0441	0.72	0.8	0.96	0.2
std-ht	$2\times 32~768~000$	116	755	0.300	0.700	0.0400	0.70	0.9	1.00	135.0
std-lt	$2\times 32~768~000$	116	755	0.300	0.700	0.0400	0.70	0.9	1.00	0.2
zoom-std-ht	$2\times 41~226~712$	3.9	25.6	0.300	0.700	0.0400	0.70	0.9	1.00	135.0

The columns (from left to right) specify: name of the run, number of particles used, gas-particle mass, dark-matter-particle mass, $\Omega_{0,{\rm m}}$ , $\Omega_{0,\Lambda}$ , $\Omega_{0,{\rm b}}$ , h, $\sigma_8$ , spectral index, star formation density threshold.

Source LaTeX | All tables | In the text

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